Environmental Engineering Reference
In-Depth Information
R
i
ε
i
B
i
Tð ð
1
k
i
W
sec
θÞþk
i
sec
θWB
i
TðÞ
(19.48)
The Planck function can be expanded into a Taylor series about the brightness
temperature
T
i
in the form of
DB
DT
T
i
BT
i
ðÞ
DB
DT
T
i
DB
DT
T
j LTðÞ
R
i
¼ B
i
TðÞ¼
j
¼
j
DB
DT
T
i
T
s
T
DB
DT
T
i
B
i
TðÞB
i
TðÞþ
j
ð
Þ
¼
j
ð
T
s
T
i
þLTðÞ
Þ
DB
DT
T
i
T
a
T
i
DB
DT
T
i
B
i
TðÞB
i
TðÞþ
j
ð
Þ
¼
j
ð
T
a
T
i
þLTðÞ
Þ
ð
19
:
49
Þ
Inserting Eq.
19.49
into Eq.
19.48
will linearize the RTE with respect to
temperature:
LTðÞε
i
1
ð
k
i
w
sec
θ
Þ T
s
T
i
þLTðÞ
ð
Þ þ k
i
w
sec
θ T
a
T
i
þLTðÞ
ð
Þ
(19.50)
Several approximations have been proposed for
L
(
T
i
). Sun and Pinker (
2003
)
use
LTðÞT
i
=n
i
(19.51)
By inserting Eq.
19.51
into Eq.
19.50
,
ð
C
i
1
T
i
ε
i
T
s
Þ ¼ T
a
ε
i
T
s
C
i
2
T
i
ð
Þ k
i
W
sec
θ
(19.52a)
where
1
þ n
i
ð
1
Þε
i
ð
n
i
1
Þ
ð
1
ε
i
Þ
C
i
1
¼
; C
i
2
¼
(19.52b)
n
i
n
i
Let
i
represent the 11.0-
μ
m channel. For most land surfaces and the ocean, the
emissivity at 11.0
m is essentially unity.
In order to reduce the number of unknown variables, we assume that the
atmospheric mean temperature
T
a
is proportional to the surface temperature
T
s
:
μ
T
a
a
w
T
s
(19.53)
It needs to be stated that assumption (
19.53
) may introduce errors if the surface
emissivity at 11.0-
μ
m channel is not close to unity. A solution for
T
s
can be obtained
as follows:
T
i
T
11
cW
sec
T
s
¼
(19.54)
½
ð
a
w
1
Þk
i
W
sec
θ þ
1
θ þ
1
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